--- license: cc-by-nc-4.0 task_categories: - image-segmentation tags: - lunar - chang-e-4 - terrain-classification - segmentation - planetary-science pretty_name: Chang'E-4 Terrain Classification Dataset --- # Chang'E-4 TCM Dataset Tools and data for terrain classification using Chang'E-4 Yutu-2 rover imagery. > **Dataset:** Segmentation masks are available on [Hugging Face](https://huggingface.co/datasets/lothanspace/change4-tcm-dataset). > **Note:** Original Chang'E-4 images are not included due to copyright restrictions. You must download the source images directly from CLPDS (see instructions below). ## Quick Start ```bash # Install dependencies pip install -r requirements.txt # Convert PDS files to images python scripts/convert_pds.py data/raw data/images ``` ## Downloading Chang'E-4 Data Data is available from China's Lunar and Planetary Data System (CLPDS). ### 1. Register an Account 1. Go to https://clpds.bao.ac.cn 2. Create an account (check spam folder for confirmation email from NAOC) ### 2. Download Data 1. Navigate to Chang'E-4 data search: https://clpds.bao.ac.cn/ce5web/searchOrder-ce4En.do 2. Select an instrument: - **PCAM** - Panoramic Camera (rover, stereo pairs) - **TCAM** - Terrain Camera (lander) - **LPR** - Lunar Penetrating Radar - **VNIS** - Visible/Near-IR Spectrometer 3. Choose data level (L2A or higher for calibrated data) 4. Add files to cart and process order 5. Download and extract to `data/raw/` ### Data Format Chang'E-4 uses PDS4 format: - XML label file (`.xml`) - metadata - Data file (`.img`, `*L`) - image data ## Converting to Images The conversion script applies debayering and contrast stretching: ```bash # Convert all PDS files in data/raw to PNG python scripts/convert_pds.py data/raw data/images # Preview files without converting python scripts/convert_pds.py data/raw data/images --dry-run # Flatten output to single directory python scripts/convert_pds.py data/raw data/images --flat ``` ### Processing Steps 1. Read PDS4 file using `pds4_tools` 2. Debayer raw Bayer images (PCAM full-resolution) 3. Apply 2% linear contrast stretch 4. Save as PNG ## Project Structure ``` ├── data/ │ ├── masks/ # Segmentation mask annotations (JSON) │ ├── raw/ # Downloaded PDS4 files (you provide) │ └── images/ # Converted PNG images (generated) ├── docs/ │ └── chinese-moon-data-access.md ├── scripts/ │ └── convert_pds.py └── requirements.txt ``` ## References - [CLPDS Data Portal](https://clpds.bao.ac.cn) - [Chang'E-4 Data Releases](https://moon.bao.ac.cn/pubMsg/detail-CE4EN.jsp) - [CLPDS Overview Paper](https://link.springer.com/article/10.1007/s11214-021-00862-3) ## Citation If you use this dataset in your research, please cite: ```bibtex @misc{chang4tcm2026, author = {Yu, Sam and Huang, Christoper and Nasika, Tanvi and Shao, Yi and Singhania, Amay}, title = {Chang'E-4 Terrain Classification Dataset}, year = {2026}, organization = {Lothan Space, IHS Maker Club}, publisher = {HuggingFace}, url = {https://huggingface.co/datasets/lothanspace/change4-tcm-dataset} } ``` Please also cite the original data source: ```bibtex @misc{clpds2025, author = {{Ground Research and Application System of China's Lunar and Planetary Exploration Program}}, title = {Chang'E-4 Scientific Data}, publisher = {China National Space Administration}, url = {https://moon.bao.ac.cn} } ``` ## License The code and segmentation masks in this repository are licensed under [CC BY-NC 4.0](LICENSE) (Creative Commons Attribution-NonCommercial 4.0). You are free to use, share, and adapt for non-commercial purposes with attribution. Original Chang'E-4 imagery is owned by CLPDS/NAOC and must be downloaded directly from their portal. See [docs/chinese-moon-data-access.md](docs/chinese-moon-data-access.md) for their citation requirements.